Proposal code
w321
Proposal title
Wiggling structure of Double Sided Jets in 0458+138
The |
Investigators and their |
Affiliations |
P.I. |
Yoshiharu Asaki |
ISAS, Japan |
|
Kenta Fujisawa |
NAO, Japan |
|
Keiichi Asada |
NAO, Japan |
|
Hideyuki Kobayashi |
NAO, Japan |
Proposal Abstract
We propose observations of 0458+138. This is a unique source having
symmetrical jets at the opposite sides of its core component.
Those jets are continuously ejected from the core.
Our main purpose of this proposal is to detect a ``wiggle-like"
structure in each of jets. In this study, we
investigate mechanisms of the accerelation and collimation of VLBI
jets. If the magnetic field is dominant to produce wiggling jets, the
wiggle pattern will show mirror-symmetry in respect with the core.
On the other hand, if the precession of an accretion disk is dominant,
the wiggle will show point-symmetry. The curving of the jets are slightly
seen in the opposite sided jets at 8.5GHz, so that VSOP observations
will reveal the wiggle-like structure of 0458+138.
The full Cover Sheets
(compressed post-script, typically 50kbytes) can
be retrieved. Note that many proposals were reduced in extent by the
Scientific Review Committee (e.g. by reducing the number of
experiments), however the Cover Sheets contain the full proposal as
submitted. Also note that AO3 proposals were submitted in October 1999,
and information such as affiliations and contact details has
changed for some proposers since that time. The Cover Sheets (and the
details on this page, which were derived from the Cover Sheets) may
therefore have changed.